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Contribution Oral
Air showers accompanied by high energy atmospheric families observed by Chacaltaya hybrid experiment
Speakers
- Dr. Masanobu TAMADA
Primary authors
- Dr. Masanobu TAMADA (Kinki University)
Co-authors
- Dr. Hiroshi AOKI (Soka University)
- Dr. Rolando TICONA (Universidad Mayor de San Andres)
- Dr. Ken HONDA (University of Yamanashi)
- Dr. Naoya INOUE (Saitama University)
- Dr. Takaaki ISHII (University of Yamanashi)
- Dr. Norio KAWASUMI (University of Yamanashi)
- Dr. Nicolas MARTINIC (Universidad Mayor de San Andres)
- Dr. Nobuaki OCHI (Yonago National College of Technology)
- Dr. Nobuharu OHMORI (Kochi University)
- Dr. Akinori OHSAWA (Institute for Cosmic Ray Research, University of Tokyo)
Abstract content
Characteristics of air-showers and accompanied high energy atmospheric families detected in the hybrid experiment at Mt. Chacaltaya are studied in detail and compared with those of simulations taking into accounts the specific detection bias of the experiment. It is shown that the observed characteristics of the atmospheric families accompanied by large air showers, Ne > 10^7, and also those of air-showers accompanying families can not be explained simply by increase of heavy nucleus in primary cosmic-rays. Discussions are also given on the comparison with the results of the other hybrid experiments on high mountains.
Reference
Proceedings of the 30th International Cosmic Ray Conference; Rogelio Caballero, Juan Carlos D'Olivo, Gustavo Medina-Tanco, Lukas Nellen, Federico A. Sánchez, José F. Valdés-Galicia (eds.); Universidad Nacional Autónoma de México, Mexico City, Mexico, 2008; Vol. 4 (HE part 1), pages 23-26